Published 1999
| Published
Book Section - Chapter
Open
Re-Accelerated Solar Wind - An Additional Source of Anomalous Cosmic Rays?
- Creators
-
Mewaldt, R. A.
- Others:
- Kieda, D.
- Salamon, M.
- Dingus, B.
Abstract
We consider the acceleration of solar, interplanetary, and interstellar particles at the solar-wind termination shock, predict expected composition and energy spectra, and discuss possible observable consequences. The acceleration of a small fraction of solar wind ions incident on the termination shock may explain low-energy enhancements in the spectra of several elements observed by Voyager beyond ~ 60 AU. Other possible particle sources are also discussed.
Additional Information
© University of Utah. Provided by the NASA Astrophysics Data System. I appreciate conversations with A. C. Cummings (who also provided numerical values for the Voyager data) and with N. Barghouty, P. C. Frisch, M. G. Baring, and J. R. Jokipii. This work was supported by NASA under NASS-30704 and NAGW-1919.Attached Files
Published - 1999-36.pdf
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Additional details
- Eprint ID
- 54827
- Resolver ID
- CaltechAUTHORS:20150213-102518440
- NASA
- NAS5-30704
- NASA
- NAGW-1919
- Created
-
2015-02-13Created from EPrint's datestamp field
- Updated
-
2019-11-22Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory